Theia 2745

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0.02 UTI
0.41
CN
0.53
Cdens
0.75
CC3
0.0
Clit
0.05
Cdup
Stellar density (N50/rad) 2.7 [N/pc2]
  • CN 0.41 Poorly populated
  • Cdens 0.53 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.05 Very likely duplicate

Overview

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Theia 2745 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 166.156 -67.539 0.932 -7.441 1.805 -6.745
Hunt & Reffert 2024 166.166 -67.522 0.924 -7.478 1.811 -8.72
Cavallo et al. 2024 166.163 -67.557 0.924 – – –
Hunt & Reffert 2023 166.166 -67.522 0.924 -7.478 1.811 -8.72

💡 Note: The UCC values are estimated from its identified members.

Reference Year Dist [kpc] Av [mag] DAv [mag] Age [Myr] [Fe/H] [dex] Mass [Msun] Bfrac BSS
UCC 99999– 1.04 0.685 0.86 108 0.340 104 – –
Hunt & Reffert 2024 – – – – – 104(1) – –
Cavallo et al. 2024 1.05 0.78 – 129 0.340 – – –
Hunt & Reffert 2023 1.03 0.59 0.86 88 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HXHWL 64 95.1 166.28 -67.58 0.93 -7.42 1.77 -5.36 0.39

💡 Note: The % column shows the percentage of members that Theia 2745 shares with each listed object.

Visualization

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